Query= T MON GCVS Query forms

NNo GCVS J2000.0 Type Max Min I Min II Epoch(JD24..) Year Period M-m/D Spectrum References Other design.

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550003 |T Mon *|062513.0+070509 |DCEP | 5.58 | 6.62 | |V |43784.615 | | 27.024649 |27 |F7Iab-K1Iab+A0V |09029 00559|

------------------------------------------------------------------------------------------------------------------------------------------------------------------ ______________The positional information: ___________________________

NNo GCVS J2000.0 p.m.(as/yr) Epoch Ident.

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550003 |T Mon |062513.00 +070508.6 |+0.003 -0.001|2000.0 | |Hip

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_______________Cross-identifications:_______________

T Mon = BD +07 1273 |

T Mon = BS 02310 |

T Mon = GSC 0145.00875 |

T Mon = HD 044990 |

T Mon = Hip 030541 |

T Mon = IRAS 06225+0706 |

T Mon = SAO 113845 |

____________________________________________________ Reference to a chart or photograph:

00559. A.Wroblewski, Urania 26, 339, 1955.

Reference to a study of the star:

09029. L.Szabados, Bud Mitt N77, 1981.

__________________________________________________________________

Remark:

    SB (Porb> = 70 yr [09397]). [A/H] = 0.3.

    There is a sguare term in the elements given in the

    Table: +5.34d*10**(-6)*E**2.

    Deviations from the parabola in the O - C, E diagram

    have a wave-like trend. If this wave is attributed to

    the light-time effect, Porb = 100 years.

    The observations are also satisfied by the following

    system of linear elements: Max = 2412874.56 + 27.0093d*E

    (JD2405200 - 15250) [09398]; Max = 2426004.62 + 27.0180d*E

    (JD2415250 - 27150); since JD2427150 -

    Max = 2436137.090 + 27.0205d*E [02392].

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